\begin{table}%t6
%\centering
\par
\caption{\label{tab:CLF}Field by field comparison of the slopes above and below
the break luminsoty ($L_{\rm b}$) for the CLFs created from freely fit spectra and the CLFs of luminosities derived from  fixed models. $L_{\rm b}$ is set to 10$^{36}$~erg~s$^{-1}$,
the slopes are for the CLF~above and below $L_{\rm b}$. Data for the bulge of M~31 comes from \cite{Shirey01} where the break is $2.5 \times 10^{36}$ erg~s$^{-1}$.}
\small  \begin{tabular}{c c c c c}
\hline \hline
Data & \multicolumn{2}{c}{Freely fit} & \multicolumn{2}{c}{Fixed model} \\
& CLF slope above $L_{\rm b}$ & CLF slope below $L_{\rm b}$ & CLF slope above $L_{\rm b}$ & CLF slope below $L_{\rm b}$ \\
 \hline 
        North~3 & 0.7 & 0.15 & 0.8 & 0.4 \\
        North~2 & 0.8 & 0.12 & 0.8 & 0.5 \\
        North~1 & 0.7 & 0.13 & 0.8 & 0.8 \\
        South 1 & 0.7 & 0.05 & 1.0 & 0.2 \\
        South 2 & 0.5 & 0.06 & 0.6 & 0.4 \\
        Bulge & 1.8(4) & -- \\ 
            \hline
          \end{tabular}
\end{table}